2013MNRAS.435.3243G


C.D.S. - SIMBAD4 rel 1.7 - 2021.04.19CEST13:53:58

2013MNRAS.435.3243G - Mon. Not. R. Astron. Soc., 435, 3243-3250 (2013/November-2)

Statistical ages and the cooling rate of X-ray dim isolated neutron stars.

GILL R. and HEYL J.S.

Abstract (from CDS):

The cooling theory of neutron stars is corroborated by its comparison with observations of thermally emitting isolated neutron stars and accreting neutron stars in binary systems. An important ingredient for such an analysis is the age of the object, which, typically, is obtained from the spin-down history. This age is highly uncertain if the object's magnetic field varies appreciably over time. Other age estimators, such as supernova remnant ages and kinematic ages, only apply to a handful of neutron stars. We conduct a population synthesis study of the nearby isolated thermal emitters and obtain their ages statistically from the observed luminosity function of these objects. We argue that a more sensitive blind scan of the Galactic disc with the upcoming space telescopes can help to constrain the ages to higher accuracy.

Abstract Copyright: © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2013)

Journal keyword(s): methods: statistical - stars: neutron - pulsars: general - stars: statistics - X-rays: stars

Simbad objects: 61

goto Full paper

goto View the reference in ADS

Number of rows : 61

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 RX J0420.0-5022 N*? 04 20 02.2 -50 22 46     25.5     ~ 82 0
2 SNR J052559-660453 SNR 05 26 00.4 -66 05 02     12.71     ~ 413 2
3 PSR B0525-66 Psr 05 26 00.7 -66 04 35           ~ 524 1
4 V* CM Tau Psr 05 34 31.93830 +22 00 52.1758           ~ 4881 1
5 M 1 SNR 05 34 31.94 +22 00 52.2           ~ 5724 4
6 PSR B0540-69 Psr 05 40 10.84 -69 19 54.2           ~ 811 3
7 RX J0720.4-3125 N* 07 20 24.961 -31 25 50.21   26.1   27.0   ~ 285 0
8 RX J0806.4-4123 N*? 08 06 23.0 -41 22 33           ~ 73 0
9 RX J0822.0-4300 X 08 22 27.00 -43 10 27.0           ~ 32 1
10 NAME Pup A SNR 08 24 07 -42 59.8           ~ 533 1
11 NAME Vela XYZ Rad 08 34.0 -45 50           ~ 1138 2
12 NAME Vela Pulsar Psr 08 35 20.65525 -45 10 35.1545     15.10     ~ 2105 1
13 NGC 3372 HII 10 45 02.23 -59 41 59.8           ~ 917 2
14 * eta Car Em* 10 45 03.5455050 -59 41 03.951060 6.37 7.034 6.21 4.90 4.41 OBepec 2262 0
15 CXOGNC J104608.71-594306.4 N*? 10 46 08.719 -59 43 06.48           ~ 17 0
16 GSH 288-00-28 sh 10 50 -59.9           ~ 3 1
17 2E 2336 HXB 10 50 08.93 -59 53 19.9           Be 385 0
18 SNR G295.5+09.7 SNR 12 09 40 -52 25.0           ~ 262 1
19 PSR J1210-5226 Psr 12 10 00.88 -52 26 28.4           ~ 210 1
20 RX J1308.8+2127 N*? 13 08 48.7 +21 27 08   28.6 28.6     ~ 146 1
21 PSR B1338-62 Psr 13 41 42.63 -62 20 20.7           ~ 117 1
22 SNR G308.8-00.1 SNR 13 42 30 -62 23.0           ~ 41 1
23 RX J1412.9+7922 X 14 12 55.885 +79 22 04.10           ~ 28 0
24 3A 1510-590 Psr 15 13 17.000 -59 04 54.00           ~ 382 3
25 PSR B1509-58 Psr 15 13 55.52 -59 08 08.8     13.06     ~ 805 1
26 RX J1605.3+3249 N*? 16 05 18.9 +32 49 07     26.8     ~ 91 1
27 PSR J1614-5048 Psr 16 14 11.29 -50 48 03.5           ~ 103 0
28 NAME ASSOC II SCO As* 16 15 -24.2           ~ 1168 1
29 SNR G332.4+00.1 SNR 16 15 20 -50 42.0           ~ 83 0
30 SNR G337.0-00.1 SNR 16 35 06.9 -47 47 25           ~ 123 1
31 GRB 980618A gB 16 35 52 -47 35.2           ~ 243 0
32 Cl Westerlund 1 OpC 16 47 04.00 -45 51 04.9           ~ 486 0
33 PSR J1647-4552 Psr 16 47 10.18 -45 52 16.7           ~ 180 1
34 SNR G343.1-02.3 SNR 17 08.0 -44 16           ~ 67 1
35 PSR B1706-44 Psr 17 09 42.7460 -44 29 07.200     13.30     ~ 590 1
36 SNR G348.7+00.3 SNR 17 13 43.0 -38 10 12           ~ 110 2
37 [AAB2008] 1 X 17 14 05.758 -38 10 31.32           ~ 51 1
38 PSR B1757-24 Psr 18 01 00.016 -24 51 27.50           ~ 220 1
39 PSR B1758-23 Psr 18 01 19.829 -23 04 44.20           ~ 128 0
40 SNR G006.4-00.1 SNR 18 01 22.7 -23 17 20           ~ 666 1
41 NAME Duck Redux Rad 18 02 10.000 -24 54 00.00           ~ 171 3
42 PSR B1800-21 Psr 18 03 51.45 -21 37 08.1           ~ 237 1
43 W 30 SNR 18 05 38 -21 36.7           ~ 160 1
44 PSR J1808-2024 Psr 18 08 39.32 -20 24 40.1           ~ 1138 2
45 PSR J1841-0456 Psr 18 41 19.29 -04 56 11.4           ~ 239 1
46 4C -04.71 Rad 18 41 19.8 -04 56 06           ~ 306 3
47 SNR G033.6+00.1 SNR 18 52 29.000 +00 38 42.00           ~ 248 1
48 PSR J1852+0040 Psr 18 52 38.49 +00 40 19.8           ~ 78 1
49 PSR B1853+01 Psr 18 56 10.65 +01 13 21.3           ~ 182 1
50 SNR G034.6-00.5 SNR 18 56 10.650 +01 13 21.30           ~ 852 2
51 RX J1856.6-3754 N* 18 56 35.11 -37 54 30.5     25.7     ~ 393 0
52 GBS 1900+14 gB 19 07 13 +09 19.6           ~ 801 0
53 PSR B1930+22 Psr 19 32 22.8562490934 +22 20 52.062067050     14.52     ~ 120 0
54 RX J2143.0+0654 N*? 21 43 03.8 +06 54 20           ~ 73 0
55 2E 4673 HXB 23 01 08.14 +58 52 44.5           ~ 597 1
56 SNR G109.1-01.0 SNR 23 01 35 +58 53.0           ~ 323 0
57 PSR B2334+61 Psr 23 37 05.779 +61 51 01.69           ~ 172 1
58 SNR G114.3+00.3 SNR 23 37 05.780 +61 51 01.69           ~ 111 1
59 NAME Gould Belt PoG ~ ~           ~ 752 1
60 NAME Magnificent Seven ? ~ ~           ~ 59 1
61 SNR G057.1+01.7 SNR ~ ~           ~ 7 0

    Equat.    Gal    SGal    Ecl

To bookmark this query, right click on this link: simbad:objects in 2013MNRAS.435.3243G and select 'bookmark this link' or equivalent in the popup menu


2021.04.19-13:53:58

© Université de Strasbourg/CNRS

    • Contact